INSTITUTE OF PHYSICS PUBLISHING JOURNAL OF PHYSICS A: MATHEMATICAL AND GENERAL J. Phys. A: Math. Gen. 37 (2004) 11547–11573 PII: S0305-4470(04)84279-3 A general stability criterion for droplets on structured substrates M Brinkmann1,2, J Kierfeld1 and R Lipowsky1 1 2 MPI für Kolloid und Grenzflächenforschung, D-14424 Potsdam, Germany Interdisciplinary Research Institute, c/o IEMN, F-59652 Villeneuve d’Ascq, France Received 2 August 2004, in final form 11 October 2004 Published 17 November 2004 Online at stacks.iop.org/JPhysA/37/11547 doi:10.1088/0305-4470/37/48/003 Abstract Wetting morphologies on solid substrates, which may be chemically or topographically structured, are studied theoretically by variation of the free energy which contains contributions from the substrate surface, the fluid– fluid interface and the three-phase contact line. The first variation of this free energy leads to two equations—the classical Laplace equation and a generalized contact line equation—which determine stationary wetting morphologies. From the second variation of the free energy we derive a general spectral stability criterion for stationary morphologies. In order to incorporate the constraint that the displaced contact line must lie within the substrate surface, we consider only normal interface displacements but introduce a variation of the domains of parametrization. PACS numbers: 02.30.Xx, 68.08.Bc, 47.20.Dr List of symbols α β δn δc1 δs2 ε θ σ ω ψ Vapour or low density phase Wetting liquid or high density phase nth variation Variation including variation of arguments on contact line Restricted second variation at a stationary shape Small real number, subscript for varied quantities Local contact angle Rigid substrate Torsion of a surface along its boundary Normal displacement field Line tension 0305-4470/04/4811547+27$30.00 © 2004 IOP Publishing Ltd Printed in the UK 11547 11548 µ A = |A | C c1 , c2 c c⊥ F F̃ F F I G g̃ gij hij Lαβσ L = |L | L∗β Lβ αβ αβσ G (s 1 , s 2 ) (t 1 , t 2 ) Sε Tε D, G ⊂ R2 M ∇ ∇2 = ∇ · ∇ N n R r t V = |V | U, V ⊂ R3 W X M Brinkmann et al Eigenvalue to second variation of free energy Surface tension Area of surface A Plane curve Principal curvatures Normal curvature, parallel to three-phase contact line Normal curvature, perpendicular to three-phase contact line Free energy, general Free energy, pressure ensemble Free energy of three-phase contact line Interfacial free energy Interval [0, Lαβσ ] Gaussian curvature Metric tensor or first fundamental form Components of metric tensor Components of extrinsic curvature tensor Three-phase contact line Length of space curve L Length scale of line tension Linear dimension of droplet Arclength parameter Width of αβ interface Width of three-phase contact line Capillary length Coordinates on αβ interface Coordinates on substrate σ Coordinates of the varied three-phase contact line Domain of parametrization Mean curvature Covariant operator Laplace–Beltrami operator Surface normal of αβ interface Conormal of the αβ interface Vector or parametrization of αβ interface Vector or parametrization of three-phase contact line Tangent of three-phase contact line Volume of spatial region V Neighbourhood Wettability of substrate σ Vector or parametrization of substrate σ 1. Introduction The morphology of droplets wetting a solid substrate is strongly influenced by topographical and/or chemical surface patterns [1]. During the past decade, much effort has been devoted, both theoretically and experimentally, to this interplay between surface structure and wetting morphologies. Experimental techniques such as micro-contact printing [2] or monolayer lithography [3] allow the fabrication of imprinted or structured planar surfaces with tailored patterns of lyophilic and lyophobic surface domains. The resulting wetting morphologies are A general stability criterion for droplets on structured substrates 11549 governed by the patterns of different wettability over a wide range of droplet volumes, as has been demonstrated in recent experiments on liquid channels [4, 5]. In these experiments, it has also been shown that an increase of the droplet volume beyond a critical value leads to a morphological transition from the liquid channel to a bulged configuration [4, 5]. Such a transition offers the possibility to fuse different microcompartments of liquid in a controlled manner, which is an attractive option for a variety of microfluidic applications [6]. The experimentally observed shapes of wetting droplets are theoretically obtained by minimizing the free energy of the droplet. In general, this free energy contains contributions from the substrate surface, from the fluid–fluid interface and from the line tension of the threephase contact line. For uniform substrate surfaces, this minimization leads to the classical equations of Laplace and Young–Dupré. For chemically and topographically structured substrate surfaces, a generalized contact line equation has been recently derived by Swain and Lipowsky [7], see further below. These two equations provide necessary conditions for the stationary configurations of the droplet but are not sufficient in order to determine whether these configurations represent minima of the free energy and thus experimentally observable shapes. Indeed, stationary droplet configurations may represent saddle points which exhibit one or several unstable directions in the free energy landscape of configurations. In order to determine the stability of a stationary droplet state, one has to study the second variation of the droplet’s free energy. The issue becomes particularly relevant at a morphological transition where two distinct shapes exchange their stability. Such morphological transitions have been found for a variety of domain patterns consisting of circular [8], striped [4, 9] and ring-shaped surface domains [10]. In the micrometre regime, the droplet shapes are governed by their interfacial free energies. Contributions arising from the three-phase contact line are expected to become relevant at a droplet size of about one hundred nanometres [1]. Thus, line tension effects are particularly relevant for small wetting structures such as liquid bridges between wetting droplets [9]. In the general framework of thermodynamics, a line contribution to the free energy of a wetting droplet is defined as an excess free energy related to the structural perturbations along the contact line [11]. Thermodynamic equilibrium implies that the interfacial tensions or free energies are always positive. In contrast, the sign of the line tension may be positive or negative [11]. Within effective interface models, the sign of the line tension is found to depend on the details of the molecular interactions as reflected in the specific form of the interface potentials, see, e.g., [12]. For uniform substrate surfaces, the equation of Young and Dupré represents the condition of mechanical equilibrium of the three-phase contact line between liquid, vapour and substrate. This equation has to be generalized for non-vanishing line tension as was first realized in [13] and extended to certain surface domain geometries in [14, 15]. More recently, Swain and Lipowsky [7] derived a rather general contact line equation which is valid for rigid substrates, both topographically and chemically structured. Several experimental studies have recently provided evidence for line tension effects on wetting phenomena [16, 17]. In [17], the line tension corrections predicted by the contact line equation in [7] have been determined by AFM measurements of the effective interface potentials close to the contact line as well as contact angle measurements on droplets with highly curved contact lines. Results derived from both methods agree and give a line tension of the order of || ≈ 10−10 J m−1 . Depending on the liquid and the substrate, is observed to have positive or negative sign [17]. In a recent experiment [18], the shape of nanometre-sized polystyrene droplets has been measured using AFM. A systematic comparison between the contact angles of droplets at different sizes shows that, in this case, the line tension attains a value of || 0.5 ×10−10 J m−1 . 11550 M Brinkmann et al In this paper, we start from basic concepts of interface thermodynamics using a general expression for the free energy of a droplet on a structured substrate including interfacial and line free energies. In the framework of differential geometry and variational calculus, we derive the first variation of the free energy and recover the general contact line equation for stationary states as previously derived by Swain and Lipowsky [7]. We then proceed to calculate the second variation of the droplet’s free energy for such a stationary configuration and, in this way, obtain a general criterion for the local mechanical stability of stationary droplet shapes. A major technical difficulty which has to be properly addressed in the variational calculation is that the contact line of the deformed droplet shape must stay within the substrate surface. In order to incorporate this constraint, previous approaches have used shape deformations of the liquid–vapour interface which were parametrized both by normal and by tangential displacements [19–21]. The tangential displacements can then be chosen in such a way that the contact line stays within the substrate surface. In this paper, we use a different calculational method for the derivation of the second variation of free energy. The shape deformations are entirely parametrized in terms of normal displacements of the initial configuration. Instead of introducing tangential displacements, the necessary shift of the contact line is incorporated by varying the domain of parametrization of the liquid–vapour interface and the wetted substrate. This scheme is rather transparent, and one can easily see how the various terms of the second variation arise from the different terms of the first variation. The paper is organized as follows. A short summary of the thermodynamic description of fluids wetting a chemically structured substrate is given in section 2. In section 3, we consider general normal displacements of the droplet shape and calculate the variations of general functionals defined on the droplet interface and contact line. The constraint that the contact line should be displaced within the substrate surface is incorporated by introducing variations of the domain of integration. In section 4, the variation of the droplet’s free energy is derived in detail. The second variation leads to a general stability criterion as shown in section 5. 2. Free energy Let us consider a droplet of a liquid β with fixed volume wetting a rigid and inert substrate σ . The wetted substrate is in contact with another third phase, denoted by α. The phase α may be a vapour phase or another liquid phase. We assume that all phases are in thermal and mechanical equilibrium. Concerning chemical equilibrium we may focus on two ideal situations that can be realized in wetting experiments: (i) The wetting phase β is non-volatile, that is, an exchange of molecules between α and β is slow on the time scale of the experiment. Since all liquids are highly incompressible at normal conditions, i.e., at temperatures and bulk pressures far from a critical point, the volume Vβ of a β droplet is virtually constant throughout the wetting process. In typical wetting experiments, the β phase may form disconnected droplets. Each β droplet attains a local minimum of the droplet’s interfacial and line free energy for its given individual volume. Due to condensation of molecules from the α phase the volume of a β droplet might increase in time and, provided that mechanical equilibration is fast, we may observe a sequence of local minima. If these conditions are fulfilled we will speak of a volume ensemble because the droplet volume represents, in principle, an accessible control parameter of the system. A general stability criterion for droplets on structured substrates 11551 (ii) The exchange of molecules between the surrounding α phase and the β droplet is fast and the system reaches chemical equilibrium. Whenever the number of particles in the α phase is much larger than in the β phase we can regard the α phase as a reservoir of molecules which fixes the chemical potential of each species in the entire system. In the case of a one-component and simple liquid β coexisting with its vapour α we are able to express the difference between the chemical potential µ, set by α, and the chemical potential µ0 at coexistence of the bulk phases by the pressure difference Pα − Pβ across the αβ interface. Thus, we refer to this situation as the pressure ensemble. In general, the free energy F of the droplet consists of different contributions related to the bulk of the droplet, its interfaces and the three-phase contact line [1]. Which of these contributions govern its morphology depends on the length scale of the droplet. Also gravitational and van der Waals forces can give relevant contributions to the free energy on large and small scales, respectively. 2.1. Interfacial and contact line energies At fixed intensive quantities the interfacial free energy F is homogeneous in the area Aij = |Aij | of each interface Aij between adjacent homogeneous phases i and j. Because of chemical inhomogeneities of the substrate walls σ , both surface tensions ασ and βσ are functions of the position X on the substrate surface Aσ . Thus, we cast the droplet’s interfacial free energy into a form F = αβ Aαβ + dA [ βσ (X) − ασ (X)], (1) Aβσ where Aβσ is the surface of σ wetted by β. To proceed with basic definitions, the three-phase contact line Lαβσ of the droplet is defined as the set of points where the αβ interface terminates on the surface of σ , i.e. Lαβσ = Aαβ ∩ Aσ . On a chemically homogeneous substrate wall the related free energy F is simply proportional to the length Lαβσ = |Lαβσ | of the three-phase contact line. However, on heterogeneous substrate walls one might expect a spatially non-uniform line tension (X) and a line integral F = dL (X) (2) Lαβσ accounts for the contact line free energy. One may also consider droplets wetting plane and homogeneous crystalline or nano-patterned surfaces where the line tension is expected to become a function of the local orientation of the contact line. The line free energy F becomes comparable with the interfacial free energy if the linear dimension, Lβ , of the droplet is of the order of the characteristic length [1] (3) L∗β = / αβ 2αβσ αβ as follows from dimensional analysis where αβ is the width of the αβ interface and αβσ is the width of the contact line. As long as the linear dimension of the droplet satisfies Lβ L∗β , the line free energy is small compared to the interfacial free energies. This does not imply, however, that the line tension has no observable consequences in this case. In fact, most estimates of the line tension are based on contact angle measurements in the regime Lβ L∗β since the contact angle is affected by the tension, see equation (64) below. The regime Lβ < L∗β may not be accessible to experimental studies if the width of the contact line is relatively small. The contact line is the intersection of three interfaces which 11552 M Brinkmann et al will, in general, differ in their width. Usually, the width of the αβ interface is comparable to the size of the molecules in the two fluid phases (exceptions are provided by phase coexistence near a critical point, where the α and β phases become indistinguishable, and by the adsorption of surfactant molecules which increase the effective interfacial width). If the substrate surface is smooth on the molecular scale, the width of the contact line should also be governed by the width of the αβ interface. In this case, the characteristic length L∗β is of the order of the molecular size as well, and droplets with linear dimensions Lβ < L∗β are not accessible. On the other hand, the magnitude of the line tension may be increased by the effect of long-range van der Waals forces. As shown in appendix E, the corresponding effective interface model leads, in the small gradient approximation, to the line tension contribution vdW ≈ 1 AH 6π θ lpin (4) from van der Waals forces. This contribution depends on the contact angle θ , the Hamaker constant AH and the wetting layer thickness l = lpin where the interface potential has a point of inflection. This line tension contribution is large for small contact angle θ , large Hamaker constant AH and small thickness lpin . A large contribution vdW increases the characteristic size L∗β ∼ , and the regime Lβ < L∗β may then become accessible. 2.2. Bulk energies The droplet’s body Vβ or, to be precise, the space occupied by the liquid β, with volume Vβ = |Vβ | is bounded by the surface Aαβ to the vapour α, and by the surface Aβσ to the rigid substrate σ , and thus, is entirely determined by the shape and position of the αβ interface. An analogue statement holds for the three-phase contact line Lαβσ and Aβσ , the surface of σ wetted by β. Hence, the droplets free energy is a functional of the αβ interface that is mathematically described by Aαβ . In order to find locally or globally stable droplet configurations in contact to the substrate walls we have to minimize the free energy F = F + F (5) under the subsidiary constraint Vβ = V allowing for a droplet volume that is equal to the value of V . The volume ensemble can be seen as analogous to a canonical ensemble since the number of particles in the incompressible phase β is fixed. Provided that, in contrast to the volume ensemble, the pressure difference P = Pα − Pβ between the fluid phases α and β is prescribed while Vβ is not fixed, i.e, the pressure ensemble applies to the system, an additional term P Vβ in the free energy F̃ = F + F + P Vβ (6) accounts for the work done or received during an exchange of volume with an external reservoir. In the volume ensemble, however, the pressure difference P is a Lagrange multiplier which has to be chosen such that the constraint of a constant volume is fulfilled. At fixed volume, the last term in (6) is a constant and does not contribute to the free energy3 . In the grand canonical ensemble, the pressure difference is fixed by the supersaturation µ = µ − µ0 with µ being the actual, fixed value of the chemical potential in the container and µ0 being the chemical potential at coexistence of bulk phases α and β. A quantitative 3 Note that P is the pressure difference between vapour α and liquid phase β which is set by the external reservoir and identical to the pressure difference across the droplet’s αβ interface if and only if the droplet is in mechanical equilibrium. A general stability criterion for droplets on structured substrates 11553 relation between the pressure difference P and the shift µ in the chemical potential at coexistence is given by the equation µ = P + O[(P )2 ], ρα0 − ρβ0 (7) with particle number densities ρi0 of phases i ∈ {α, β} at bulk coexistence. Gravity does not affect the shape of droplets which are significantly smaller than the capillary length 2 αβ , (8) G = a(ρβ − ρα ) where relevant contributions to the droplet free energy come from the interfaces and, for droplets in the submicrometre regime, from the three-phase contact lines between adjacent bulk phases [1]. Effects of gravity can be eliminated on a macroscopic length scale performing wetting experiments with two liquids of nearly the same mass densities ρα and ρβ as well as in space crafts or drop towers where the acceleration a is typically reduced by a factor of 10−4 to 10−6 compared to normal conditions on earth. The capillary length G is typically of the order of millimetres or even larger. 3. Droplet shape Small deformations of a liquid droplet β that is freely suspended in a fluid α can be represented by normal displacements of the αβ interface with respect to the initial droplet configuration. However, normal displacements are not sufficient to describe deformations of a droplet β wetting the wall of a substrate σ . The shift of the contact line under general shape variations may have a tangential component with respect to the αβ interface. One obvious way to approach this problem is to introduce an additional displacement along a tangential direction close to the boundary of the αβ interface as first introduced in [19]. The tangential shift together with the normal displacement allows for the constraint of a contact line gliding on the substrate walls. Within such an approach, it is hard to eliminate the tangential displacement field in the final results. It seems that this problem has been overcome in [20, 21] where displacement fields for each order of the variational problem have been introduced including a tangential shift. Due to the constraint of a gliding contact line these fields are not independent and subject to a condition that is derived in a long calculation in [21]. This condition can be employed to eliminate tangential components in the final expressions for free energy variations. In this paper, we use a different approach to treat the constraint of the contact line gliding on the walls of the substrate σ . By constructing an extension of the αβ interface beyond the surface of σ and by use of special coordinate systems close to the contact line we were able to vary the domains of parametrizations of the αβ interface and of the surface of σ that is wetted by β, respectively. This approach turns out to be computationally advantageous as it naturally leads to the occurrence of boundary terms in the variations of physical quantities, like interfacial energies or droplet volume. As we will show in the following, it enables us to split up the variations into terms which are entirely related to either the variation of the αβ interface or the variation of the contact line. This justifies a classification of these variations into ‘surface’ and ‘boundary’ terms which will be marked with superscripts (s) and (b), respectively. 11554 M Brinkmann et al 3.1. Parametrizations It is reasonable to assume that the substrate wall σ , the droplet’s αβ interface and three-phase contact line are smooth, that is, they exhibit no edges or kinks. The αβ interface of the droplet, we denote by Aαβ , is parametrized by smooth functions R = (R 1 , R 2 , R 3 ) with x = R(s 1 , s 2 ) (9) in local coordinates (s 1 , s 2 ) ∈ D ⊂ R2 that are mapped onto Euclidean vectors x = (x 1 , x 2 , x 3 ) ∈ Aαβ ⊂ R3 . A tangential plane to a given point of Aαβ is spanned by a pair of linearly independent tangent vectors Ri = ∂R/∂s i for any regular parametrization. √ By convention, the local normal vector N = (R1 × R2 )/ g on Aαβ points from the√liquid √ β to the vapour α. In the definition above we used the local surface element g = det g of the metric tensor g, or first fundamental form, with components gij = Ri · Rj . Within the formalism of co- and contravariant components, elements of the matrix inverse g −1 of g will be written as (g −1 )ij = g ij in local coordinates. The surface area of Aαβ is measured by an integral √ Aαβ = dA = d2 s g, (10) Aαβ D which is invariant under reparametrizations of the αβ interface. The surface Aβσ , i.e., the part of the surface of σ wetted by the liquid β, is parametrized by smooth functions X = (X1 , X2 , X3 ) with x = X(t 1 , t 2 ) (11) in local coordinates (t , t ) ∈ G ⊂ R and with a three-dimensional Euclidean vector x ∈ Aβσ ⊂ R3 . Trivially, an inclusion Aβσ ⊂ Aσ holds with the surface of σ here denoted by Aσ . Tangent vectors Xi = ∂X/∂t i define the metric tensor components gij∗ = Xi · Xj and a √ √ √ local surface element g ∗ = det g ∗ . A corresponding normal vector M = (X1 × X2 )/ g ∗ on Aβσ points from the substrate σ to the liquid β. We will use the convention that all quantities or operators referring to Aβσ or Aσ are marked with a star to distinguish them from those defined on Aαβ . The three-phase contact line Lαβσ = Aαβ ∩ Aσ , i.e, the set of points where the liquid β, the vapour α and the substrate σ meet can be described as the rim of either the surface Aαβ or Aβσ . Smooth functions r = (r 1 , r 2 , r 3 ) represent the contact line as a space curve 1 2 x = r() 2 (12) with ∈ I ⊂ R and x ∈ Lαβσ ⊂ R3 . By reparametrization one may choose the parameter such that || is identical to the arclength on the contact line. Hence, we have I = [0, Lαβσ ] with Lαβσ , the length of the contact line. Apart from the local tangent t = ṙ/|ṙ| to Lαβσ we will use a conormal vector n = t × Nc to the surface Aαβ which forms a right-handed local frame (n, t, Nc ) of R3 in every point of Lαβσ . Here and below, we denote the total derivative with respect to the parameter by a dot. The vector Nc is the local surface normal N of Aαβ restricted to points of Lαβσ . Provided that the boundary curve r() has a positive orientation with respect to the surface normal N the conormal n points outwards when seen from Aαβ . A conormal m = t × Mc to the surface Aβσ yields a second orthonormal and right-handed frame (m, t, Mc ) of R3 with Mc , the surface normal M of Aβσ restricted to points of Lαβσ . The local contact angle θ between Aαβ and Aβσ is defined by a scalar product cos θ = n · m = Nc · Mc , (13) A general stability criterion for droplets on structured substrates 11555 (α) N Mc c θ m t n (β) (σ) Figure 1. Cut through a droplet β on a substrate σ , perpendicular to the contact line Lαβσ . The droplet β is surrounded by a vapour phase α. In points on Lαβσ we denote the surface normal of the αβ interface Aαβ by Nc and the surface normal to the substrate Aσ by Mc . The outward-pointing normal n is perpendicular to t and Nc yielding a local orthonormal local frame of R3 . The local frame (n, t, Nc ) on Aαβ is tilted by the local contact angle θ against the corresponding local frame (m, t, Mc ) on Aσ . as illustrated in figure 1. The relative orientation of Aαβ and Aβσ with respect to the parametrization of Lαβσ implies that n = m and Nc = Mc provided θ = 0 holds. By the divergence theorem one can rewrite the droplet volume as a surface integral over Aαβ and Aβσ . We have 1 1 Vβ = dV = dA R · N − dA X · M 3 Aαβ 3 Aβσ Vβ 1 1 √ = d2 s g R · N − d2 t g ∗ X · M, (14) 3 D 3 G which turns out to be a computationally advantageous starting point when varying the αβ interface. The signs in front of the first and the second term are due to the different orientations of the normal N to Aαβ and the normal M to Aβσ when seen from the bulk of β. 3.2. Extending surfaces We are able to construct a small stripe Sαβ along the contact line Lαβσ that provides a smooth continuation A¯αβ = Aαβ ∪ Sαβ of the αβ interface beyond the contact line, see also appendix A. Here, the term ‘smooth’ means in particular that the normal curvature is defined in any point and along any direction in the corresponding local tangential plane on the extended surface A¯αβ . A continuation A¯βσ = Aβσ ∪ Sβσ of the wetted surface of σ can be easily constructed since Aβσ is embedded in the smooth substrate wall Aσ . Both continuations are necessary to account for variations in the position of the contact line under small deformations of the droplet. It is convenient to introduce special parametrizations x = R(s 1 , s 2 ) on A¯αβ and x = X(t 1 , t 2 ) on A¯σβ in the vicinity of Lαβσ , for details see appendix A. Given a parametrization of Lαβσ as a space curve x = r() we have r() = R(S(), ) = X(T (), ), (15) with s = S() = 0, t = T () = 0 and s = t = for all ∈ I . As the second coordinate is now given by the parameter we may introduce the simplifying notation s = s 1 and t = t 1 that is clear as long as we refer to this special coordinate system. 1 1 2 2 11556 M Brinkmann et al Both coordinate systems arise naturally in the construction of the extensions that we outline in appendix A. The absolute value |s| is the arclength on a coordinate line defined by = const between a particular point x = R(s, ) and the contact line. The point x will be located on the extending stripe Sαβ if the coordinate s satisfies the inequality 0 s < S̄(), and x will lie on Aαβ if s < 0 holds. The rim of the extending stripe is parametrized in these coordinates by a function s = S̄(). Analogue statements hold for the extending stripe Sβσ and coordinates (t, ) of A¯βσ . Here, the rim of the extending stripe is given by a function t = T̄ (l) in local coordinates. Now, for the domains of parametrization D ⊂ R2 and G ⊂ R2 with Aαβ = R(D) Aβσ = X(G ), we can find extended domains D̄ ⊂ R2 and G¯ ⊂ R2 such that A¯αβ = R(D̄) A¯βσ = X(G¯). (16) (17) Expressed in the special coordinates the domains parametrizing the extending stripes Sαβ and Sβσ assume the particular form D̄\D = [0, S̄] × I G¯\G = [0, T̄ ] × I . (18) As shown appendix A the local tangent t to the contact line satisfies t = R2 |s=0 = X2 |t=0 , (19) i.e, is identical to the second local tangent vector on the αβ interface and of the surface of σ wetted by β, respectively, in points on the contact line. The remaining tangent vectors R1 |s=0 = n X1 |t=0 = m (20) in points on the contact line represent the local conormal n to the αβ surface and the local conormal m to the wetted surface of σ , respectively. 3.3. Variation of shape To test for stationarity or local stability of the αβ interface we have to impose small deformations to the αβ interface before calculating changes in the interfacial free energy. Given a parametrization R of the extended αβ interface A¯αβ we represent the varied, extended αβ interface (A¯αβ )ε by x = Rε (s 1 , s 2 ) = R(s 1 , s 2 ) + δR(s 1 , s 2 ), (21) 3 1 2 ¯ )ε ⊂ R . We choose a displacement δR = εψN along with (s , s ) ∈ D̄ and x ∈ (Aαβ the surface normal N of the unvaried surface A¯αβ where ψ(s 1 , s 2 ) is a smooth function of coordinates s i on the extended surface A¯αβ and ε is a small and real number. Now, in order to describe the physical part of the varied αβ interface (Aαβ )ε ⊂ (A¯αβ )ε , the domain of parametrization D is varied to Dε ⊂ D̄ with (Aαβ )ε = R(Dε ) ⊂ (A¯αβ )ε . The latter inclusions presuppose that |ε| is sufficiently small. This procedure can be seen as cutting off the redundant part of the varied extended αβ interface that is lying in the bulk of the substrate σ . The remaining physically relevant part (Aαβ )ε of the αβ interface is bounded by the varied contact line (Lαβσ )ε that is defined by the relation (Lαβσ )ε = (Aαβ )ε ∩ Aσ . Under the shift of the contact line, the surface of σ that is wetted by β has to be varied to (Aβσ )ε = X(Gε ) ⊂ A¯βσ with a corresponding varied domain Gε ⊂ G¯. It is one of the central issues of this paper to calculate the variation of the domains D and G of parametrization from this geometrical constraint. Equation (15) serves as a starting point to determine the coordinates of the varied contact line. This condition can be rewritten as rε () = Rε (Sε (), ) = X(Tε (), ) (22) A general stability criterion for droplets on structured substrates 11557 in coordinates s = Sε () and t = Tε () of the varied contact line (Lαβσ )ε on the varied extended αβ interface (A¯αβ )ε and the extended wetted surface A¯βσ of σ , respectively. The varied domains of parametrization Dε and Gε are expressed in the form D̄\Dε = [Sε , S̄] × I G¯\Gε = [Tε , T̄ ] × I (23) using the special coordinate systems. Differentiation of equation (22) with respect to the small parameter ε yields with equation (20) the relation (24) δ 1 r = nδ 1 S + Nc ψ = mδ 1 T . d 1 The notation δ (·) = dε (·) ε=0 is an abbreviation for the first variation of a function under the deformation of the αβ interface. By subsequent scalar multiplication of equation (24) with n, Nc and m, and by comparison with the definition of the local contact angle θ defined in (13) we find ψ δ 1 S = ψ cot θ δ1T = δ 1 r = mδ 1 T , (25) sin θ where all quantities refer to the unvaried contact line. The requirement of smooth curvatures on the contact line, as guaranteed by continuation of the αβ interface described in the preceding section and appendix A, ensures that the variations (25) are uniquely defined. 3.4. Surface and boundary terms As a first application of formula (25) we will calculate the variation of a general class of functionals √ E {Aαβ } = dA E = d2 s gE, (26) Aαβ D that depend on the configuration Aαβ of the αβ interface. The geometrical quantity E defined on the extended surface A¯αβ is a function of local coordinates (s 1 , s 2 ) ⊂ D̄. Note that the first and the second variation of the functional Eε = E {(Aαβ )ε } which depends on the real number ε through the varied αβ interface (Aαβ )ε are defined by dEε d2 Eε 1 2 δ E= . (27) δ E {ψ} = dε dε2 ε=0 ε=0 In particular, this definition implies that the iterated first variation is identical to the second variation δ 1 (δ 1 E ) = δ 2 E . To continue, we calculate the first variation of E as the first derivative d √ 1 2 √ δ E {ψ} = d s gε Eε = d2 s δ 1 ( g)E dε D D ε=0 ε d √ 2 1 2 √ 2 √ d s gδ E + d s gE − d s gE . (28) + dε D Dε D ε=0 The last term in the general expression (28) comes from the variation of the domain of parametrization (23) which is due to the shift of the contact line. In the special coordinate system defined in section 3.2 and using first variations as given in (25) we may expand the first coordinate of the contact line as Sε = εψ cot θ + O(ε2 ) around ε = 0. By construction of √ the coordinate system we have g = 1 + O(s) around s = 0, as follows from (19) and (20). The last term of (27) leads to a ‘boundary’ term d √ √ d2 s gE − d2 s gE δ 1 E b {ψ} = dε Dε D ε=0 Sε d √ = d ds gE = d E cot θ ψ. (29) dε I 0 ε=0 I 11558 M Brinkmann et al to the first variation of the functional E . The remaining terms in (28) give rise to a ‘surface’ term √ 1 s 2 1√ δ E {ψ} = d s δ ( g)E + d2 s gδ 1 E. (30) D D Note that this surface term would be zero if the surface Aαβ itself were not varied. We conclude that an equivalent surface term in the first variation of an analogous class of functionals E ∗ {Aαβ } = dA E ∗ = d2 t g ∗ E ∗ , (31) Aβσ G which are defined as an integral over the surface of σ wetted by β, is absent, i.e., we have δ 1 E ∗ s {ψ} = 0. (32) Here, we use an expansion Tε = εψ/ sin θ + O(ε ) of the first coordinate of the varied contact line around ε = 0 to show that the boundary term to the first variation of the functional (31) is given by d 1 ∗b 2 ∗ 2 ∗ ∗ ∗ ds g E − d t g E δ E {ψ} = dε Gε G ε=0 Tε d Eψ . (33) = d dt g ∗ E ∗ = d dε sin θ I 0 I ε=0 √ An expansion g ∗ = 1 + O(t) can be performed around t = 0, as follows again from relations (19) and (20). To proceed with the computation of the surface term (30), we calculate the first variation √ δ 1 ( g) of the local surface element using the Gauss–Weingarten map which assumes the form 2 j ∂i N = hi Rj (34) in local coordinates. We find local tangent vectors to the varied αβ interface j (Rε )i = Ri + Rj hi εψ + Nε∂i ψ, (35) j hi of the extrinsic curvature tensor are positive on a where, in our definition, all elements spherical surface. From equation (35) we derive the expression (gε )ij = gij + 2hij εψ + O(ε2 ) (36) for the varied components (gε )ij of the metric tensor gij , and we are able to compute the first √ variation of the local surface element g. Given a non-singular matrix a and an arbitrary matrix b, the useful identity d det(a + εb)|ε=0 = Tr(a −1 b) det(a) (37) dε allows us to calculate a directional derivative of a determinant. By use of formula (37) and the expansion (36) we obtain √ √ √ δ 1 ( g) = ghii ψ = 2 gMψ (38) i as the first variation of the local surface element. The trace M = hi 2 is the mean curvature and equals the mean value of the two principal curvatures. Since the trace of the extrinsic curvature tensor is invariant under any reparametrization which conserves the orientation of the surface, the mean curvature represents a local geometrical invariant of a surface [22]. Inserting equation (38) into the surface term (30) and with the boundary term (29) we arrive at a general expression dA 2MEψ + dA δ 1 E + dL E cot θ ψ (39) δ 1 E {ψ} = Aαβ Aαβ Lαβσ A general stability criterion for droplets on structured substrates 11559 for the first variation of the functional E which itself is a functional of the normal displacement field ψ on A¯αβ . The first variation of the analogous functional E ∗ {Aαβ } of the wetted surface of σ , however, is given by a boundary term E∗ψ . (40) dL δ 1 E ∗ {ψ} = sin θ Lαβσ Finally, we compute the variation of a general class of functionals B which are defined as an integral over the contact line. Since the substrate σ is rigid and thus its surface is not varied the contact line is entirely determined by the shape and position of the αβ interface. Dropping, for the moment, the assumption that is an arclength parameter on the contact line we may write B{Aαβ } = dLB = d|ṙ|B, (41) Lαβσ I where B is a function of local geometrical quantities. These quantities, for instance, depend on the position on the varied αβ interface and on the surface of σ and, hence, change under a shift of the contact line. The variation of the functional B leads to two terms d|ṙ|δc1 B + d δc1 (|ṙ|)B, (42) δ 1 B{ψ} = I I where the first term arises from the variation of the geometrical quantity that is due to the variation of the αβ interface and the accompanying shift of the contact line. The subscript c indicates a total variation under the shift of the contact line including all arguments. The second term describes the effect of local lengthening or shortening of the contact line under the normal displacement by ψ. The first variation of the line element becomes ṙ · δ 1 ṙ = t · (ṁδ 1 T + mδ 1 Ṫ ), (43) |ṙ| where we used the identity (24) and the Leibnitz rule. With the definition of the geodesic curvature ṫ · m t · ṁ cg∗ = =− (44) |ṙ| |ṙ| of the contact line with respect to the surface of σ and the orthogonality relation m · t = 0 we can rewrite expression (43) as cg∗ ψ δc1 (|ṙ|) = t · ṁδ 1 T = |ṙ| . (45) sin θ The first variation of the functional B is then given by cg∗ Bψ 1 1 , (46) δ B{ψ} = dL δc B + sin θ Lαβσ δc1 (|ṙ|) = where we still have to compute the total variation δc1 B of the integrand B while allowing for the tangential shift of the contact line. First, we consider the situation where the integrand B depends on the position of the contact line on the varied extended αβ interface and the surface of σ , i.e., on the functions Sε () and Tε (). Since, by definition, the second coordinate is not varied, we have dBε (Sε , Tε , ) δc1 B = = δ 1 B + (∂s B)δ 1 S + (∂t B)δ 1 T (47) dε ε=0 for the total first variation of the integrand B due to the variational shift of the contact line. The first variation of the coordinates of the contact line, δ 1 S and δ 1 T , is given in (25). 11560 M Brinkmann et al In the other situation, the integrand B does not depend on the position of the contact line but on the direction of the contact line on the substrate wall, i.e., on the unit vector m. This situation is of interest when considering homogeneous but anisotropic substrates σ . For simplicity, we assume that the anisotropic surface of σ is planar so that we can describe the orientation by a single angle φ between the conormal m and a fixed unit vector e lying in the plane of the surface, i.e., cos φ = m · e. This leads to a first variation δc1 (cos φ) = −sin φδc1 φ = e · δc1 m. (48) The first variation of the conormal is calculated in appendix C with the result δc1 m = −tδ 1 Ṫ for a planar substrate, see equation (C.16). By the simple relation sin φ = −t · e we conclude that δc1 φ = −δ 1 Ṫ . We are now able to calculate the first variation of the quantity B under the rotation of the contact line induced by the shift. Instead of relation (47) being valid for a spatially dependent B we now have δc1 B = dBε (φε ) = δ 1 B − (∂φ B)δ 1 Ṫ dε ε=0 (49) for the total first variation of an integrand B due to the rotation of the contact line under the variation. 4. Variation of free energy Using the results for the variation of generic functionals derived in the preceding section we will now calculate first and second variations of the interfacial free energy and line energy for droplets wetting a rigid substrate wall. The result for the second variation is valid only for stationary droplet shapes but this restriction may be of no significance since applied to test for local stability. In the pressure ensemble, a stationary configuration of the αβ interface is reached whenever the first variation of the total free energy vanishes under any small deformation. In contrast, for non-volatile and incompressible droplets the volume ensemble holds and thus a constraint of a constant volume has to be imposed on the class of configurational variations of the αβ interface. In principle, the conditions of stationarity do not reveal any information about the local or global stability of the droplet. The volume term in the free energy (6) can be seen, depending on the ensemble, either as a Langrangian term or as an energy term that accounts for the exchange of volume with an external reservoir. This observation implicates that the set of stationary configurations with fixed volume and the set of stationary configurations at fixed Laplace pressure are identical. But because of the constraint of constant volume, the set of locally mechanically stable configurations in the pressure ensemble is a subset of all locally mechanically stable configurations in the volume ensemble. In what follows, we will focus our attention mostly on the volume ensemble. As opposed to local stability, global stability can only be inferred if all branches of stationary configurations in the wetting geometry are known. Wetting geometries which allow such an exhaustive analytical solution of the first variational problem are rare and, in many cases, exhibit non-analytical solutions as well. In a numerical investigation, this has been demonstrated by Lenz and Lipowsky for droplets wetting a planar lyophobic substrate which is decorated with a lyophilic ring [10]. A general stability criterion for droplets on structured substrates 11561 4.1. First variation A general expression of the first variation including both interfacial free energy and line free energy has been derived by Swain and Lipowsky [7]. The condition for a mechanical equilibrium of the αβ interface is still given by the equation of Laplace while the equation of Young–Dupré has to be modified due to line tension. Effects of line tension are strong whenever the curvature of the contact line is large, as it is the case for small droplets, or if the line tension depends strongly on the position on the substrate. Already some decades ago, Gretz considered the equilibrium shape of small spherical droplets on a chemically homogeneous substrate including line tension [13]. He derived a quantitative expression for the deviation of the local contact angle at mechanical equilibrium of a small droplet from a macroscopic droplet. Our calculation, however, allows us to consider the first variation of arbitrarily shaped droplets. As introduced in section 2 we write the free energy of small droplets in the form F̃ = F + F + P Vβ , (50) where the influence of gravity has been neglected. We assume, for the moment, that the droplet exchanges volume with an external reservoir at a given pressure difference P = Pα − Pβ between the fluid phase α and the wetting liquid β. If we do not allow changes in the droplet volume Vβ the last term in the free energy (50) becomes a constant. In this case P can be seen as a Lagrange multiplier, see section 2. According to equation (1) we split the interfacial free energy F into the free energies Fαβ and Fβσ , which are related to the αβ interface and the surface of σ wetted by β, respectively. The variation of the interfacial free energy Fαβ = αβ Aαβ can be performed with the general expression (39) for the particular case E = 1 which leads to surface and boundary contributions s b {ψ} + δ 1 Fαβ {ψ} δ 1 Fαβ {ψ} = δ 1 Fαβ dA 2Mψ + = αβ Aαβ dL cot θ ψ . (51) Lαβσ On the other hand, the interfacial free energy which stems from the wetted part of σ is given by an integral dAW, (52) Fβσ = − αβ Aβσ where the wettability W = ( ασ − βσ )/ αβ ranges between −1 and 1. As the variation of the αβ interface leaves the shape of the rigid substrate σ unchanged we find no surface s = 0, see (32). Therefore, the only contribution contribution to the first variation, i.e., δ 1 Fβσ to the first variation of the interfacial free energy Fβσ is due to the boundary and obtained by setting E ∗ = W in equation (33) as Wψ b . (53) {ψ} = − dL δ 1 Fβσ {ψ} = δ 1 Fβσ sin θ Lαβσ Another contribution to the total free energy of the droplet comes from line tension and, thus, is sensitive to the variation of the three-phase contact line only. According to equation (46) the first variation of the line energy (2) consists of two terms cg∗ ψ . (54) dL δc1 + dL δ 1 F {ψ} = sin θ Lαβσ Lαβσ 11562 M Brinkmann et al The first term in (54) describes variations of the line energy which emerge from a positional change of the contact line and the chemical inhomogeneity on the surface of σ . Applying equation (47) we find δc1 = (∂t )δ 1 T = ψm · (∇ ∗ ) , sin θ (55) where we used the covariant derivative ∇ ∗ = Xi ∂i defined on the extended surface A¯βσ . The first variation of the line energy is then given by ψ 1 (cg∗ + m · ∇ ∗ ). δ F {ψ} = dL (56) sin θ Lαβσ The last term of the free energy F̃ in the volume ensemble contains the volume Vβ of the liquid droplet. By definition the pressure difference P is fixed by the external volume reservoir and, thus, is not varied. A variation of the droplet volume can be easily performed in the representation by surface integrals (14) with the result 1 1 ψ 1 1 1 dA(N · δ R + δ N · R) + dL r · (cos θ Nc − Mc ) δ Vβ {ψ} = , (57) 3 Aαβ 3 Lαβσ sin θ where we applied the identities (15), (39) and (40). The varied αβ interface is represented through normal displacements, and following equation (21) we have δ 1 R = ψN. The first variation of the normal N to the αβ interface is given by the simple expression δ 1 N = −∇ψ, as shown in appendix B, see equation (B.5). Here, ∇ = Ri ∂i is the covariant derivative on the extended surface A¯αβ . Then, by use of Gauss theorem − dA R · ∇ψ = dA ψ∇ · R − dL n · rψ (58) Aαβ Aαβ Lαβσ on Aαβ and employing the identity ∇ · R = R · Ri = = 2 we arrive at the first variation 1 ψ 1 . (59) dA ψ + dL r · (Nc cos θ − n sin θ − Mc ) δ Vβ {ψ} = 3 Lαβσ sin θ Aαβ i δii The vector decomposition Mc = Nc cos θ − n sin θ (compare figure 1) on the contact line shows that the boundary term of the first variation is zero. Hence, we find a first variation of the droplet volume that is simply given by δ 1 Vβ = δ 1 Vβs = dA ψ, (60) Aαβ and has no boundary term. Collecting the terms from the first variations of the free energies of the αβ interface (51), the wetted surface of σ (53), the line energy (56) and the droplet volume (60) we finally arrive at the expression δ 1 F̃ {ψ} = δ 1 F {ψ} + δ 1 F {ψ} + P δ 1 Vβ {ψ} dA(2 αβ M + P )ψ = Aαβ + dL Lαβσ ψ [ αβ (cos θ − W ) + cg∗ + m · ∇ ∗ ] sin θ (61) as the first variation of the droplet free energy in the pressure ensemble which consists of a surface and a line integral. Since the normal displacement field ψ on the αβ interface is arbitrary, we can infer from the condition δ 1 F̃ {ψ} = 0 of mechanical equilibrium that the A general stability criterion for droplets on structured substrates 11563 arguments of both the surface integral and the line integral in (61) have to vanish identically. This leads to the equation of Laplace 2 αβ M = −P = Pβ − Pα on Aαβ , (62) and the generalized equation of Young and Dupré αβ cos θ = ασ − βσ − cg∗ − m · ∇ ∗ on Lαβσ (63) for stationary droplet shapes. The latter result was obtained first in its general form by Swain and Lipowsky [7]. Here, the local equilibrium contact angle θ is not only a function of the position, but also depends on the orientation m and geodesic curvature cg∗ of the contact line with respect to the surface of the substrate. In the following, we will briefly discuss the somewhat different situation of a homogeneous and planar, but anisotropic surface of a crystalline or nanopatterned substrate σ . The conormal m and a fixed direction e on the surface of σ form an angle φ which was already introduced in (3.4). A variation of the line energy now leads to 1 (64) dL[cg∗ δ 1 T − (∂φ )δ 1 Ṫ ], δ F = Lαβσ where the dot denotes a derivative with respect to an arclength parameter on the contact line. Note that on a planar surface of σ we find a relation cg∗ = φ̇. By a partial integration with respect to the arclength parameter for a closed (or periodic) contact line on the planar surface we arrive at the first variation dL cg∗ + ∂φ2 δ 1 T , (65) δ 1 F = Lαβσ and the following generalization of the equation of Young and Dupré: αβ cos θ = ασ − βσ − cg∗ + ∂φ2 on Lαβσ . (66) It may happen on a surface of a crystalline or periodically nanopatterned substrate that the second derivative ∂φ2 becomes large and positive for certain contact line orientations. Since the cosine of the contact angle ranges between −1 and 1 the geodesic curvature cg∗ of the contact line with respect to the surface of σ has to go to small positive values in a small range of orientations which leads to a strong faceting of the droplet’s three-phase contact line. Such faceting effects have recently been observed for liquid alloy droplets wetting a Si surface [23]. 4.2. Second variation The second variation of the free energy can be obtained by iterated variation of the result (61) for the first variation. Although the calculation is in principle straightforward using the techniques we have provided for treating boundary terms arising from the contact line, a much simpler expression for the second variation can be obtained if we restrict ourselves to the calculation of the second variation for stationary droplet shapes for which the first variation has to vanish. Consequently, the conditions of Laplace (62) and Young–Dupré (63) have to be fulfilled. In the following, we will write for the ‘restricted second variation’, i.e., the second variation evaluated at a stationary shape, the symbol δs2 (.) to distinguish from the ordinary operator δ 2 (.) of second variation. Then, we obtain from iterated variation of the first variation (61) at such a stationary shape the expression dA ψδ 1 (2 αβ M + P ) δs2 F̃ {ψ} = Aαβ + dL Lαβσ ψ 1 δ [ αβ (cos θ − W ) + c∗ + m · ∇ ∗ ]. sin θ c (67) 11564 M Brinkmann et al The final result for the restricted second variation has a much simpler form compared to the full second variation because the arguments in the surface and in the line integral of (61) are zero in any point of the αβ interface and contact line, respectively, for a stationary droplet shape. Hence, variations of the domain of integration and the variation of the local surface or line element need not be considered in (67). Using the result (B.12) for the first variation of the mean curvature we find 2 s dA 2ψδ 1 M δs F̃ {ψ} = αβ Aαβ = αβ Aαβ dA ψ[−∇ 2 + (2G − 4M 2 )]ψ (68) as the surface contribution to the restricted second variation of the free energy in the pressure ensemble. The second-order differential operator ∇ 2 = ∇ · ∇ is the Laplace–Beltrami operator on A¯αβ . The second term in (67) gives the boundary contributions to the restricted second variation and leads to four terms: the first term describes the variation of the local contact angle θ under the deformation of the αβ interface; a second term arises from the position-dependent wettability W on the substrate and the shift of the contact line; the third and the fourth term are related to the change of the geodesic curvature and the position-dependent line tension. Expressed in an orthonormal coordinate system, as given by the special coordinate systems close to the contact line introduced in section 3.2, the co- and the contravariant components of any tensor become identical and the components of the curvature tensor can be identified with local normal curvatures or torsions of the surface in the directions of the coordinate lines. In the following, we will denote the components of the extrinsic curvature tensor on the contact line by special symbols. In particular, we use c⊥ = h11 for the normal curvature of the αβ interface perpendicular to the contact line, ω = h12 = h21 for the torsion or winding of the αβ interface along the contact line, and c = h22 for the normal curvature parallel to the ∗ , ω∗ and c∗ are introduced with respect to the special contact line. Corresponding symbols c⊥ orthonormal coordinate system on the surface of σ . Employing the general result for the first total variation (47) of a quantity defined on the contact line and from the definition of the local contact angle (13) we find cos θ Mc · ∂s N + Nc · ∂t M ψ, (69) δc1 (cos θ ) = Mc · δ 1 N + sin θ where the first variation δ 1 N and the derivatives ∂s N and ∂t M are taken on the contact line. By use of the Gauss–Weingarten equation (34) together with (19) and (20), the first variation of the surface normal (B.5), and some trigonometry the above expression simplifies to ∗ − c⊥ cos θ )ψ. δc1 (cos θ ) = sin θ n · ∇ψ + (c⊥ (70) A further contribution to the second term in the restricted second variation of the free energy (67) arises from a position-dependent wettability W of the substrate wall. The first variation under the shift of the contact line is simply given by ψm · ∇ ∗ W . (71) sin θ Whenever we deal with large droplets of linear dimension Lβ L∗β , line energies become irrelevant, and we can neglect all terms which contain the line tension . In this case, the boundary contribution to the restricted second variation of the free energy reduces to dL ψ( αβ n · ∇ + u )ψ, (72) δs2 F b {ψ} = δc1 W = (∂t W )δ 1 T = Lαβσ A general stability criterion for droplets on structured substrates coming from the interfacial energies where u denotes the expression ∗ c⊥ m · ∇∗ W − c⊥ cot θ − , u = αβ sin θ sin2 θ 11565 (73) ∗ defined on the contact line and depending on normal curvatures c⊥ and c⊥ as well as the derivative of the wettability W in the direction of the conormal m. If we consider the local stability of small droplets with linear dimension in the range Lβ L∗β we have to include the remaining last two terms in (67), both related to line energy, into our consideration. Iterated variation leads to the restricted second variation ψ 1 δ (m · ∇ ∗ + cg∗ ). δs2 F {ψ} = dL (74) sin θ c Lαβσ The first term can be further transformed into δc1 (m · ∇ ∗ ) = ∇ ∗ · δc1 m + m · (∇ ∗ ⊗ ∇ ∗ ) · mδ 1 T , (75) containing the first variation of the conormal with respect to the surface of σ . The second term leads to two new terms δc1 (cg∗ ) = δc1 cg∗ + cg∗ m · (∇ ∗ )δ 1 T , (76) which account for the variation of geodesic curvature cg∗ and the coupling of the geodesic curvature to the position-dependent line tension . The lengthy calculations of the first variation of the geodesic curvature cg∗ and the first variation of the conormal m with respect to the substrate are presented in appendix C with the result (77) δc1 cg∗ = −δ 1 T̈ − cg∗ 2 + G∗ δ 1 T and δc1 m = −t δ 1 Ṫ − Mc cg∗ δ 1 T . The first variation of the two bracketed terms in expression (74) becomes ˙ 1 Ṫ δc1 (m · ∇ ∗ + cg∗ ) = −δ 1 T̈ − δ ∗ + cg m · ∇ ∗ + m · (∇ ∗ ⊗ ∇ ∗ ) · m − cg∗ 2 + G∗ δ 1 T . (78) (79) Recalling that the first factor in (74) is simply given by ψ/ sin θ = δ 1 T we may perform a partial integration in the parameter along the closed contact line which yields a symmetric representation 2 dL[(δ 1 Ṫ )2 + v(δ 1 T )2 ] (80) δs F {ψ} = Lαβσ of the restricted second variation of the line energy where v is an abbreviation for v = cg∗ m · ∇ ∗ + m · (∇ ∗ ⊗ ∇ ∗ ) · m − cg∗ 2 + G∗ . (81) In a similar manner, the surface term of the second variation (68) assumes a symmetric form after an integration by parts which eliminates the term ψn · ∇ψ under the line integral in (72). Including both the interfacial and the line energy contributions, the restricted second variation of the free energy of a droplet wetting a rigid substrate σ can be cast into the final form dA[(∇ψ) · (∇ψ) + (2G − 4M 2 )ψ 2 ] δs2 F̃ {ψ} = αβ Aαβ dL + Lαβσ (ψ̇ − θ̇ ψ cot θ )2 + (v + u sin2 θ )ψ 2 , sin2 θ (82) 11566 M Brinkmann et al where the functions u and v , defined by (73) and (81), respectively, depend on the normal ∗ as well as on the geodesic curvature cg∗ of the contact line and the curvatures c⊥ and c⊥ ∗ Gaussian curvature G with respect to the surface of σ , and derivatives of the wettability W and line tension in the direction of the conormal m. The restricted second variation (82) of the droplet’s free energy is the main result of this paper. It agrees with the result given in [20] with details of its derivation in [21]. As expected, expression (82) is symmetric in the displacement field ψ on the αβ interface. Note also that we have eliminated the pressure difference P in equation (82) as the restricted second variation is taken at a stationary configuration and as we have implicitly made use of the Laplace equation (62). In the case of a uniform line tension, the function (81) depends only on the line tension and on the intrinsic curvature of the substrate wall and contact line, that is, the Gaussian curvature G∗ and the geodesic curvature cg∗ . Introducing ripples to the boundary of the αβ interface lengthens the contact line as indicated by the first term in the boundary integral (82). This term has the same sign as the line energy. 5. Spectral stability criterion The second variation of the free energy of a locally stable droplet has to be non-zero and positive for any deformation of the αβ interface that is compatible with the constraint of a constant droplet volume. Hence, positivity of the restricted second variation δs2 F̃ {ψ} implies local stability of the droplet. The final, symmetric form (82) shows that the restricted second variation of the free energy is a quadratic form in the displacement field ψ and positivity can be inferred from its spectrum of eigenvalues µ on the subspace of volume-conserving displacements ψ. The smallest eigenvalue yields the desired information about local stability. A droplet configuration is locally stable if and only if the smallest eigenvalue is positive. The spectrum of eigenvalues can be found by diagonalizing the quadratic form δs2 F̃ {ψ} on the subspace of volume-conserving displacements ψ using the well-known extremal property of eigenfunctions, which establishes the equivalence to an eigenvalue problem for a partial differential equation with specific boundary conditions [24]. For non-volatile and incompressible liquids, the droplet volume has to be conserved under any deformation of the αβ interface. For the stability analysis of configurations that are stationary under such a constraint we have to test the restricted second variation (82) for positivity on a subspace of displacements that enforces the volume-constraint up to linear order in ψ as shown in appendix D. The expression of the first variation of the droplet volume (57) shows that this condition is equivalent to dA ψ = 0, (83) δ 1 Vβ {ψ} = Aαβ which defines a linear subspace U⊥ of all displacement fields on the αβ interface. The displacement field is normed by dA ψ 2 = 1, (84) Aαβ and all fields ψ that satisfy (84) are said to belong to the unit sphere S of elongation fields on the αβ interface. Now, the quadratic form δs2 F̃ {ψ} can be diagonalized by extremizing on the restricted set S of normalized displacement fields ψ on the αβ interface [24]. The associated Lagrange A general stability criterion for droplets on structured substrates 11567 multiplier for the restriction to S is the eigenvalue µ. For non-volatile liquids with conserved volume, further restriction of S to the subset S⊥ = S ∩ U ⊥ of fields has to be considered in the stability analysis instead of S . Equivalently, we can introduce another Lagrange multiplier ν, and find that the quadratic form δs2 F̃ {ψ} is diagonalized by displacement fields ψ which are local extrema of the functional Q{ψ} = δs2 F {ψ} − µ Aαβ dA ψ 2 − ν dA ψ, (85) Aαβ where, so far, no restrictions are made upon ψ. Both parameters µ and ν have to be chosen such that the subsidiary conditions of normalization (84) and of conserved volume (83) are satisfied for an extremal field ψ. The extremizing displacement field ψ is an eigenfunction in the subspace of volume-conserving displacements ψ, and the parameter µ the corresponding eigenvalue of the second variation δs2 F {ψ} restricted to U⊥ . We finally conclude after a partial integration of the symmetric form Q{ψ} that the extremal condition δ 1 Q{ψ} = 0 is equivalent to the inhomogeneous version of a partial differential eigenvalue equation −∇ 2 ψ + (2G − 4M 2 )ψ = µψ + ν on Aαβ . (86) The partial integration of Q{ψ} further shows that the displacement field ψ has to fulfil a linear boundary condition v 1 + u ψ + r{ψ} = 0 on Lαβσ , n · ∇ψ + (87) αβ sin2 θ where the function r{ψ} on the contact line has a form d d ψ 1 . (88) r{ψ} = − αβ sin θ d d sin θ If the smallest eigenvalue µ to a solution ψ of the partial differential equation (86) with boundary condition (87) is positive, the restricted second variation (82) is also positive, which implies local stability of the stationary configuration. A uniform local contact angle θ and line tension in (88) yields the simplified expression r{ψ} = −ψ̈/( αβ sin2 θ ), which applies to simple droplet morphologies on plane substrates with uniform wettability and line tension, as we will consider in a following publication. 6. Conclusion In this work, we have derived the most general form of the second variation (82) of the free energy for a stationary droplet wetting a rigid substrate with spatially heterogeneous surface topography, wettability and line tension. A new variational technique was introduced to treat the motion of the contact line under arbitrary deformations of the droplet’s liquid– vapour interface. Within this variational technique it is sufficient to consider only normal displacements of the liquid–vapour interface. Using this formalism, we are able to recover expression (61) for the first variation of the free energy which has been obtained previously by Swain and Lipowsky [7] and leads to a generalized equation of Young and Dupré (63) for heterogeneous substrates including line tension effects. We have also considered the situation of a homogeneous but anisotropic line tension for a planar substrate. In this case, we obtain expression (65) for the first variation of the free energy and a different generalization (66) of the equation of Young and Dupré which can give rise to a faceting of wetting morphologies. Starting from the result (82) for the restricted second variation we derived the partial differential equation (86) with boundary conditions (87) which allows a systematic stability analysis of stationary droplet shapes and will be applied to a simple wetting geometry in a following publication. 11568 M Brinkmann et al t Figure 2. Illustration of the construction of the extending stripes Sαβ and Sβσ . As outlined in appendix A we construct an array of planes P perpendicular to the tangent t of Lαβσ . Provided that the contact line Lαβσ is smooth the planes P do not intersect each other in a sufficiently small neighbourhood U(x) around a point x ∈ Lαβσ . Our variational scheme may be useful in a variety of other contexts. Possible applications include the stability analysis of fluid membrane vesicles adsorbed onto a substrate with spatially heterogeneous chemical composition. Due to the presence of additional bending energies, an expression for the second variation of the elastic free energy for a fluid membrane that includes all boundary contributions is much harder to obtain and remains an open problem to which the variational technique developed in this paper might be successfully applied. Appendix A. Coordinates and extending stripe A smooth extension of the αβ interface can be constructed in the following way. At first, we consider an array of planes where each plane P is perpendicular to the tangent t of the contact line Lαβσ in the point of intersection, see figure 2. Furthermore, each plane P intersects the surface Aαβ in the vicinity of Lαβσ and generates a curve Cαβ = P ∩ A αβ which ends on Lαβσ . Since the planes do not intersect each other in a sufficiently small neighbourhood U(r0 ) ∈ R3 of a given point r0 ∈ Lαβσ , any point x ∈ Aαβ ∩ U(r0 ) belongs to exactly one curve Cαβ . In the next step, each curve Cαβ of intersection will be continued by a small piece of a circular arc C¯αβ ⊂ P pointing in the direction of the conormal n of the interface Aαβ . The curvature of the arc C¯αβ shall be identical to the curvature c⊥ in the end point of Cαβ on Lαβσ . Hence, Cαβ ∪ C¯αβ is a smooth curve in the plane P perpendicular to t as indicated in figure 2. Finally, by collecting all curves C¯αβ into a stripe Sαβ we have constructed a regular extension of the surface Aαβ in a sufficiently small neighbourhood of r0 . In order to show this proposition we parametrize the contact line by an arclength parameter and the curve Cαβ ∪ C¯αβ by the arclength parameter s. The coordinates s shall satisfy s > 0 on the continuation C¯αβ , s < 0 on Cαβ , and consequently s = 0 on Lαβσ . Since by definition, the conormal n and the tangent t of the contact line Lαβσ are orthonormal we can argue by continuity that the tangent vectors R1 and R2 are linearly independent in a sufficiently small neighbourhood V(r0 ) ⊂ U(r0 ). Smoothness of the extended surface A¯αβ = Aαβ ∪ Sαβ is guaranteed by the construction and the fact that n, t and c⊥ are smooth functions of the arclength parameter on Lαβσ . A general stability criterion for droplets on structured substrates 11569 Appendix B. Variation of surface normal and mean curvature We will start our calculation with the variation of the surface normal N of the αβ interface. As N · N = 1 we find N · δ 1 N = 0. (B.1) Variation of the orthogonality relation Ri · N = 0 gives 0 = δ 1 Ri · N + Ri · δ 1 N = ∂i ψ + Ri · δ 1 N, (B.2) where we used (35). Due to (B.2), we can make an ansatz δ 1 N = a j Rj (B.3) for the variation of the surface normal with numerical coefficients a j . These coefficients can be determined by inserting the ansatz (B.3) into (B.2), which leads to a j = −g ij ∂i ψ. (B.4) We obtain the final result δ 1 N = −Rj g ij ∂i ψ = −Ri ∂i ψ = −∇ψ, (B.5) where ∇ = Ri ∂i is the covariant operator on A¯αβ . As expected, δ 1 N is oriented perpendicular to the unit surface normal N of the αβ interface. Using the covariant operator ∇ = Ri ∂i , the mean curvature M can be expressed as 2M = ∇ · N = Ri · ∂i N, (B.6) which leads directly to a first variation 2δ 1 M = δ 1 Ri · ∂i N + Ri · ∂i (δ 1 N). (B.7) From variation of the orthogonality relation Ri · Rj = δji we conclude δ 1 Ri · Rj = −Ri · δ 1 Rj and by use of expression (34) we arrive at j j δ 1 Ri · ∂i N = δ 1 Ri · Rj hi = −δ 1 Rj · Ri hi . (B.8) The relation R · N = g Rj · N = 0 provides together with the first variation (35) a further transformation into i ij j j j δ 1 Ri · ∂i N = −Rk · Ri hi hkj ψ − N · Ri hi ∂j ψ = −hi hij ψ. (B.9) By explicit calculation one may check that the double sum can be rewritten as j −hij hi = 2G − 4M 2 . (B.10) Together with (B.5) the second term on the right-hand side of equation (B.7) yields the simple expression Ri · ∂i (δ 1 N) = −Ri · ∂i Rj ∂j ψ = −∇ 2 ψ, (B.11) with the Laplace–Beltrami operator ∇ 2 = ∇ · ∇ on the A¯αβ . Finally, we arrive at the first variation δ 1 M = − 12 ∇ 2 ψ + (G − 2M 2 )ψ of mean curvature. (B.12) 11570 M Brinkmann et al Appendix C. Variation of conormal and geodesic curvature To compute the first variation of the conormal m, we make an ansatz δc1 m = am m + at t + aM Mc , (C.1) with three unknown coefficients am , at and aM . Scalar multiplication of (C.1) with m and using the variation of m · m = 1 gives the first coefficient am = m · δc1 m = 0. (C.2) By scalar multiplication of equation (C.1) with t and, again, using the variation of an orthogonality relation t · m = 0 we find at = t · δc1 m = −m · δc1 t, (C.3) where the first variation of the tangent vector δc1 t = δc1 (ṙ/|ṙ|) = m δ 1 Ṫ + ṁ δ 1 T − t cg∗ δ 1 T (C.4) can be calculated using (43). To proceed, we make an ansatz for the derivative of the conormal ṁ = bm m + bt t + bM Mc (C.5) with coefficients bm , bt and bM and find the first and the second coefficient to be bm = m · ṁ = 0 and bt = t · ṁ = cg∗ . (C.6) Using the orthogonality Mc · m = 0 the third coefficient can be transformed into bM = Mc · ṁ = −Ṁc · m. (C.7) c The total derivative of the surface normal M of the substrate σ on the contact line with respect to the arclength is given by Ṁc = m ω∗ + t c∗ , (C.8) where ω∗ is the torsion along the contact line and c∗ the normal curvature parallel to the contact line. Thus, we have bM = −ω∗ (C.9) for the third coefficient and consequently ṁ = t cg∗ − Mc ω∗ . (C.10) Inserting the relation above into equation (C.4), the first variation of the tangent becomes δc1 t = mδc1 ṫ − Mc ω∗ δ 1 T . (C.11) Consequently, the second coefficient in the ansatz (C.1) is at = −δ 1 Ṫ . (C.12) The third and the last coefficient can be transformed into aM = δc1 m · Mc = −m · δc1 Mc . (C.13) The first variation of the surface normal to the substrate σ under a variation of the contact line is ∗ 1 δ T, δc1 Mc = mc⊥ (C.14) and we finally arrive at ∗ 1 δ T. aM = −c⊥ (C.15) A general stability criterion for droplets on structured substrates 11571 Reinserting all coefficients back into ansatz (C.1) gives ∗ 1 δc1 m = −t δ 1 Ṫ − Mc c⊥ δ T (C.16) for the first variation of the conormal m to the wetted surface of σ . Our next task will be to calculate the variation of the geodesic curvature cg∗ with respect to the surface of σ . By the use of (43) and the definition (44) of the geodesic curvature we have δc1 cg∗ = −m · δc1 ṫ − ṫ · δc1 m − cg∗ 2 δ 1 T . (C.17) From the orthogonality t · Mc = 0, we can easily derive ṫ · Mc = −t · Ṁc = −c∗ (C.18) and end up with ∗ 1 ∗ ∗ 1 −ṫ · δc1 m = ṫ · Mc c⊥ δ T = −c⊥ c δ T (C.19) for the second term on the right-hand side of equation (C.17). In order to calculate the first term, we derive the first variation of the tangent vector (C.11) with respect to the arclength parameter, yielding δc1 ṫ = ṁ δ 1 Ṫ + m δ 1 T̈ − (m ω∗ 2 + t c∗ ω∗ + Mc ω˙∗ )δ 1 T and eventually, after scalar multiplication with the conormal m, the relation −m · δc1 ṫ = ω∗ 2 δ 1 T − δ 1 T̈ . (C.20) Using the definition of the Gaussian curvature ∗ ∗ G∗ = c⊥ c − ω∗ 2 on the surface of σ in points of the contact line we finally arrive at δc1 cg∗ = −δ 1 T̈ − cg∗ 2 + G∗ δ 1 T (C.21) (C.22) for the first variation of the geodesic curvature of the contact line with respect to σ . Appendix D. Volume constraint for stationary droplet configurations If we like to enforce the volume constraint up to a second order in ε we have to introduce a normal variation of the αβ interface δR = (εψ + ε2 φ)N (D.1) with fields ψ and φ such that δ 1 Vβ {ψ} = 0 in a linear order and δ 1 Vβ {φ} + δ 2 Vβ {ψ} = 0 in quadratic order in the small parameter ε. Inserting the field χ = ψ + εφ into an expansion of the free energy F̃ = F̃0 + δ 1 F̃ {χ }ε + 12 δ 2 F̃ {χ }ε 2 + O(ε 3 ) (D.2) and rearranging the terms in powers of ε shows that only the field ψ appears in the quadratic order of the expansion (D.2) of the free energy F̃ as long as the preceding linear term vanishes. Hence, it is sufficient to enforce the volume constraint up to a linear order if we like to consider the restricted second variation (82) for stationary droplet configurations in the volume ensemble. 11572 M Brinkmann et al Appendix E. Van der Waals contribution to line tension In this appendix, we will briefly consider the wetting of homogeneous substrate surfaces in the presence of van der Waals forces. Such interactions can be included in the framework of effective interface models which include long-ranged interface potentials [1, 25]. In general, van der Waals forces may favour incomplete or complete wetting corresponding to non-zero and zero contact angle, θ , respectively. For partial wetting and non-zero contact angle, these forces are described by an attractive interface potential U (l) which has a minimum at l = lmin and decays as AH 1 U (l) ≈ (E.1) 12π l 2 for large l with the Hamaker constant AH [26]. Such an interface potential must also have a point of inflection which we denote by l = lpin . The potential depth Umin ≡ U (lmin ) is related to the interfacial free energies via |Umin | = αβ + βσ − ασ = αβ (1 − cos(θ )) ≈ 12 αβ θ 2 where the asymptotic equality reflects the small gradient expansion. Within this effective interface model, the line tension is given by ∞ lpin U (l) ≈ 2 αβ dl U (l) + |Umin | + dl √ . U (l) + |Umin | lpin lmin (E.2) (E.3) The first integral represents the contribution from the short-ranged forces as previously discussed in [1]. The second integral represents the contribution from the long-ranged forces. If we insert the asymptotic behaviour U (l) ≈ AH /(12π l 2 ) and the small gradient expression |Umin | ≈ 12 αβ θ 2 into the second integral, we get the line tension contribution vdW ≈ 1 AH 6π θ lpin (E.4) from the van der Waals forces. This contribution becomes large in the limit of small contact angles θ , i.e., in the limit of complete wetting. For θ 1/6π 3◦ , this line tension contribution satisfies vdW AH / lpin . References [1] [2] [3] [4] [5] [6] [7] [8] [9] [10] [11] [12] [13] [14] [15] [16] [17] [18] Lipowsky R, Lenz P and Swain P S 2000 Colloids Surf. A 161 3 Xia Y and Whitesides G M 1998 Angew. Chem. Int. Ed. 37 550 Burmeister F, Schäfle C, Matthes T, Böhmisch M, Boneberg J and Leiderer P 1997 Langmuir 13 2983 Gau H, Herminghaus S, Lenz P and Lipowsky R 1999 Science 283 46 Darhuber A A, Troian S M, Miller S M and Wagner S 2000 J. Appl. Phys. 87 7768 Whitesides G M and Stroock A 2001 Phys. 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